Novel Impedance-Matching Method for Plasma Processing at Very High Frequency Band

1996 ◽  
Vol 35 (Part 1, No. 9A) ◽  
pp. 4799-4806 ◽  
Author(s):  
Takeshi Aoki ◽  
Kazuaki Fukasawa ◽  
Yasuo Nishikawa ◽  
Nobuo Mikoshiba
1991 ◽  
Vol 58 (9) ◽  
pp. 986-987 ◽  
Author(s):  
H. Ikezi ◽  
J. S. DeGrassie ◽  
J. Drake

2020 ◽  
Vol 30 (11) ◽  
pp. 1909501 ◽  
Author(s):  
Akifumi Yamamura ◽  
Takaaki Sakon ◽  
Kayo Takahira ◽  
Takahiro Wakimoto ◽  
Mari Sasaki ◽  
...  

2010 ◽  
Vol 25 (11n12) ◽  
pp. 922-935 ◽  
Author(s):  
WEI-TOU NI

In this paper we first present a complete classification of gravitational waves according to their frequencies: (i) Ultra high frequency band (above 1 THz); (ii) Very high frequency band (100 kHz–1 THz); (iii) High frequency band (10 Hz–100 kHz); (iv) Middle frequency band (0.1 Hz–10 Hz); (v) Low frequency band (100 nHz–0.1 Hz); (vi) Very low frequency band (300 pHz–100 nHz); (vii) Ultra low frequency band (10 fHz–300 pHz); (viii) Hubble (extremely low) frequency band (1 aHz–10 fHz); (ix) Infra-Hubble frequency band (below 1 aHz). After briefly discussing the method of detection for different frequency bands, we review the concept and status of space gravitational-wave missions — LISA, ASTROD, ASTROD-GW, Super-ASTROD, DECIGO and Big Bang Observer. We then address to the determination of dark energy equation, and probing the inflationary physics using space gravitational wave detectors.


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